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Data: Stellar Quadrant Observations – 5/31/19

Yesterday promised a beautiful night. Temperatures in the low 70’s falling to mid 60’s overnight, clear skies, and no moon. So I packed up the quadrant and met Hugo at Brommelsiek to do some observing.

Unfortunately, despite the skies being clear, there was a lot of humidity and spotting stars past 3rd magnitude was challenging. Hugo was only able to stay a little over an hour, but I stayed out almost 4, and only had 15 observations at the end of the night.

As usual, details below the fold. Continue reading “Data: Stellar Quadrant Observations – 5/31/19”

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Almagest Book III: Table of the Mean Motion of the Sun

To help us determine where the sun is on a given date, Ptolemy sets out a table to allow us to more quickly look this up instead of needing to calculate how far around the ecliptic the sun has moved. This table is very similar to another set of tables Ptolemy would produce later: The Handy Tables. However, there are some notable differences between this table and the Handy Tables. Continue reading “Almagest Book III: Table of the Mean Motion of the Sun”

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Almagest Book III: On the Length of the Year

If I were to summarize the books of the Almagest so far, I’d say that Book I is a mathematical introduction to a key theorem1 and an introduction to the celestial sphere for the simplest case of phenomenon at sphaera recta. In Book II, much of that work is extended to sphaera obliqua, but in both cases, we’ve only dealt with more or less fixed points on the celestial sphere: The celestial equator, ecliptic, and points within the zodiacal constellations based on the immovable stars.

But the ultimate goal of the Almagest and my project isn’t to study the unchanging sky; it’s to understand the changing sky: The sun, moon, and planets. Ptolemy decides to start with the position of the sun is a prerequisite to understanding the phases of the moon, and planets are more complicated with their retrograde motions. And to kick off the investigation of the motion of the sun, Ptolemy first begins by carefully defining a “year” noting

when one examines the apparent returns [of the sun] to [the same] equinox of solstice, one finds that the length of the year exceeds 365 days by less than $\frac{1}{4}$-day, but when one examines its return to the fixed stars, it is greater [than 365 $\frac{1}{4}$-days].

Continue reading “Almagest Book III: On the Length of the Year”

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Data: Stellar Quadrant Observations – 5/17/19

Last night was a full moon which meant observing would be challenging, but the weather was too nice, and we’re in the season in which it’s sufficiently rare that I’m not at an event on a given weekend, so I couldn’t pass up observing. This time I was joined by his Excellency Josef von Rothenburg and his eldest daughter Maggie. As usual, observing details below the fold. Continue reading “Data: Stellar Quadrant Observations – 5/17/19”

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Almagest Book II: Table of Zenith Distances and Ecliptic Angles

Finally we’re at the end of Book II. In this final chapter3, Ptolemy presents a table in which a few of the calculations we’ve done in the past few chapters are repeated for all twelve of the zodiacal constellations, at different times before they reach the meridian, for seven different latitudes.

Computing this table must have been a massive undertaking. There’s close to 1,800  computed values in this table. I can’t even imagine the drudgery of having to compute these values so many times. It’s so large, I can’t even begin to reproduce it in this blog. Instead, I’ve made it into a Google Spreadsheet which can be found here.

First, let’s explore the structure.

Continue reading “Almagest Book II: Table of Zenith Distances and Ecliptic Angles”

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Almagest Book II: Angle Between Ecliptic And Altitude Circle – Calculations

In the last post, we started in on the angle between the ecliptic and an altitude circle, but only in an abstract manner, relating various things, but haven’t actually looked at how this angle would be found. Which is rather important because Ptolemy is about to put together a huge table of distances of the zenith from the ecliptic for all sorts of signs and latitudes. But to do so, we’ll need to do a bit more development of these ideas. So here’s a new diagram to get us going.

Here, we have the horizon, BED. The meridian is ABGD, and the ecliptic ZEH. We’ll put in the zenith (A) and nadir (G) and connect them with an altitude circle, AEG4. Although it’s not important at this precise moment, I’ve drawn it such that AEG has E at the point where the ecliptic is just rising. Continue reading “Almagest Book II: Angle Between Ecliptic And Altitude Circle – Calculations”

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Data: Stellar Quadrant Observations – 5/4/19

This year has been pretty rough for observing. With the quadrant being damaged and having to toss out a night of data in February, combined with cloudy weather in March and April, I haven’t been able to get much done.

But last night the weather cooperated and I was able to take the quadrant out, this time with the assistance of Megan doing the recording, and me doing the sighting. While I’m still not as good as Padraig, the results were fairly good and posted below the fold.

Continue reading “Data: Stellar Quadrant Observations – 5/4/19”

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Almagest Book II: Angle Between Ecliptic And Altitude Circle – Relationships

We’re almost to the end of book II. There’s really 2 chapters left, but the next one is almost entirely a table laying out the values we’ve been looking at here recently, so this is the last chapter in which we’ll be working out anything new.

In this chapter, we’ll tackle the angle between the ecliptic and a “circle through the poles of the horizon”. If you imagine standing outside, the zenith is directly overhead which is the pole for your local horizon. Directly opposite that, beneath you, is the nadir. If these two points are connected with a great circle, that’s the great circle we want to find the angle of with respect to the ecliptic. Because we measure upwards, from the horizon, along an arc of these great circles, to measure the altitude of a star, these are often called altitude circles.

But while we’re at it, Ptolemy promises that we’ll also determine “the size of the arc…cut off between the zenith and…the ecliptic.” In other words, because the ecliptic is tilted with respect to the horizon, the arcs between the two will be different.

To get us started, Ptolemy begins with the following diagram.

Continue reading “Almagest Book II: Angle Between Ecliptic And Altitude Circle – Relationships”